README web version of /home/usg/OPS/MTS/readme_xml/readme_78505304
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
These are the last MIDI observations of the Nova V1280 Sco.
The N band magnitude of the source has brightened to reach about 6O Jy, and the
flux should be close to its maximum. The correlated flux has decreased with the
increase of the angular diameter of the source but it is not a limiting factor.
The observations should be performed within the 3 weeks from now, when the N band
flux is still high.
The source is now as extended as 15mas and can be resolved by any baseline from
32 to 90m, but in order to keep the consistancy with the previous observations a
baseline between 40 and 70m is preferred. There is no need of a specific PA angle
but the largest PA coverage would provide the best constraints on the source putative
asymetry.
All the technical coordinators of this DDT proposal are warmly thanked for the success
of these observations.
Waiver Requests
Critical Observing Condition Constraints
Time-Critical Aspects
Special Execution Requirements
Special Calibration Information
ToO Information
ToO Activators List
Is this a Pre-imaging run ?
Pre-imaging Requirements
Source(s) of Pre-imaging
Pre-imaging sources not listed above
Do all your OBs comply with the instrument-specific requirements listed
on the instrument-specific Phase 2 web page ?
If this is a pre-imaging run, did you select PRE-IMAGING for the Observing
Category for each Observing Template ?
Do all your finding charts comply with both the general and instrument-specific
Phase 2 Web Pages ?
If you submitted OBs for standard stars, did you specify the magnitude
and spectral type of all standard stars in the OBs ?
Have you included OBs for any calibrations that you need but which are
not part of the Calibration Plan ?
If you are observing Moving Targets, have you attached suitable ephemeris
files to your OBs?
If you have preferences which OBs should be executed first, did you make
use of the User Priority field in the OBs ?
If this is a run that requires coordinated observations with other facilities,
did you give proper instructions in the Time-Critical Aspects Section ?
Did you indicate for each science star OB the corresponding calibrator
star OB (and vice versa) in the 'Instrument Comments' field ?
Did you check that your chosen calibrator is bright enough for the instrument
mode used ?
If you use calibrator stars which are not in the CalVin database, did
you specify their characteristics in the README file and in the OBs ?
Last creation of page: Tue Oct 6 15:40:17 2009
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